The Radial Velocity Method for Finding Exoplanets

Credit: ESO/L. Calçada. This animation shows how astronomers use very precise spectrographs to find exoplanets. As the planet orbits, its gravitational pull causes the parent star to move back and forth. This tiny radial motion shifts the observed spectrum of the star by a correspondingly small amount because of the Doppler shift. With super-sensitive spectrographs, the shifts can be measured and used to infer details of a planet’s mass and orbit.